There
are more atoms in a human eye than there are stars in the entire
universe. So we learn in the opening moments of the sixth episode of
Cosmos, “Deeper, Deeper,
Deeper Still”. One of the most mesmerizing things about Cosmos
is the way it draws together the commonalities between the cosmic and
atomic scales—the awe-inspiringly huge and the equally
awe-inspiringly tiny. It takes two things that people generally think
of as separate and unconnected and shows how they’re both part of
the same cosmos. Each affects the other, and we can never have a full
understanding of one without having an understanding of the other.
While this episode’s focus is on the atomic realm, it must still
look to the stars in order to explain it all.
The
episode takes us first on a journey into the microscopic realm of a
dew drop, introducing us to the tiny lifeforms that live there, such
as the tardigrade, one of the most resilient creatures in the world.
We then enter plant cells to learn about the workings of
photosynthesis to produce energy. There’s some rather entertaining
computer animation imagining the inner workings of the cells as a
factory production line, almost steampunk-like in its presentation.
It’s a little odd, to be sure, but it helps to simplify a complex
process that is still not fully understood. As Neil deGrasse Tyson
narrates, we can recreate photosynthesis in a laboratory, but with
nowhere near the efficiency and precision of an actual plant cell. If
we could, we would solve all the world’s energy problems. And as
unusual as the factory-like animation may seem, it’s important to
remember that most of the animation in this series is simplified to
make it easier for viewers to digest. The representation of atoms in
this episode and others, for example, is not really what atoms look
like, but they provide a useful, easily comprehended stand-in for
actual atoms. One of the goals of Cosmos is
to entrance new people into the scientific fold, to inspire future
scientists—and inspiring the series has certainly managed to be!
Following
the steampunk plant cells, the episode proceeds to take us deeper
still into the worlds of molecules and atoms. We learn of the carbon
atom and its formation into complex molecules that allow life itself.
We learn a little more of evolution, particularly the development of
our ability to smell and just what scent actually is (collections of
molecules with specific shapes that receptors in our noses register).
And we go even deeper into the nucleus of the atom and its
surrounding shell of electrons.
This
episode doesn’t stop with just the structure of the atom, however.
It also looks at one of the most populous yet elusive particles in
the universe, the unbelievably tiny neutrino. I was mesmerized by the
trip inside the Super-Kamioka Neutrino Detection Experiment in Japan.
As Tyson says about neutrinos, “The lengths one must go to track
them down is nothing short of astonishing.” I’ve known of what
must be done to detect neutrinos, but have never actually seen it
before. Combined with the knowledge of how neutrinos can pass through
virtually anything, it becomes truly awesome.
Like
other Cosmos episodes,
“Deeper, Deeper, Deeper Still” doesn’t just tell us the
science. It also provides the history behind it, from the Greek
philosopher Democritus who first postulated the existence of atoms,
to Darwin who postulated the existence of the long-tongued
sphinx-moth, to Wolfgang Pauli who postulated the existence of the
neutrino. The history helps enlighten us not just to who did what,
but to how. Tyson
explains the law of conservation of energy and how an apparent
violation of that law led Pauli to conceive of the existence of a
neutrino well before we actually found proof of it, much like Darwin
predicted the sphinx-moth fifty years before it was discovered, and
Democritus predicted the atom centuries before proof of its existence
was found. Cosmos
shows us how science can be used to extrapolate and predict with
incredible accuracy things that we have not yet discovered.
And
like most Cosmos episodes,
this one also leaves us with several things that we don’t yet have
the answers for. We learn how studying neutrinos might allow us to
see past the “Wall of Forever” into the origins of the universe.
That unbelievably tiny particle, smaller even than an electron, may
hold secrets to the entirety of the universe. It takes us right back
to the idea that the incredibly big and the incredibly small are all
just a part of the same thing. We are all star stuff.
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